Complement to VIII/85A

Source WN_B1447.2+3801B: points from spectra and waste tables

  Postscript Figure Additional frequencies and fluxes in ν and S Data as a Table  
Adapt
Plot
nu
S
x cuts: xlog Bitmap size:
y cuts: ylog
"-c="

The 2 columns in color are computed by VizieR, and are not part of the original data.
The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/spectra
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
The parameters of the radio spectra[image][spectrum] (631736 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq n a b RAJ2000 DEJ2000 MHz mJy mJy arcsec [mJy] deg deg
74 VLSS J1449.2+3748 2.19e+03 4.4e+02 79.98 65273 0 -1.11 5.52 222.3221 +37.8144 151 6C 144718+380124 1.45e+03 2.9e+02 252.00 65273 0 -1.11 5.51 222.3208 +37.8167 151 7C 144718.19+380105.00 1.27e+03 2.5e+02 70.20 65273 0 -1.11 5.52 222.3212 +37.8114 232 MY 144718.1+374847.7 5.10e+02 1.0e+02 150.00 65273 0 -0.94 4.96 222.3208 +37.8133 325 WN B1447.2+3801 6.59e+02 1.3e+02 12.00 65273 0 -1.11 5.52 222.3194 +37.8145 325 WN B1447.2+3801B 6.07e+02 1.2e+02 12.00 65273 0 -1.11 5.51 222.3211 +37.8122 365 TXS 1447+380 6.57e+02 1.3e+02 6.00 65273 0 -1.11 5.51 222.3209 +37.8123 408 B2.3 1447+38 3.85e+02 7.7e+01 0.00 65273 0 -1.11 5.52 222.3158 +37.8133 408 B3 1447+380 4.20e+02 8.4e+01 84.00 65273 0 -1.11 5.52 222.3212 +37.8150 1400 NVSS J144917+374843 1.16e+02 2.3e+01 45.00 65273 0 -1.11 5.51 222.3209 +37.8120 4730 B3a 1447+380 2.80e+01 5.6e+00 168.00 65273 0 -1.14 5.64 222.3212 +37.8151 4850 GB6 B1447+3801 3.78e+01 7.6e+00 108.00 65273 0 -1.14 5.64 222.3117 +37.8222 10600 B3VLA 948 1.00e+01 2.0e+00 69.00 65273 0 -1.11 5.52 222.3208 +37.8117

The column SED is a link to a plot of the radio spectrum, and the column Radio+Opt is a link to an Aladin preview. The SED plot contains points from the cross-identification (spectra; red), from the waste basket (waste; yellow), and the fitted radio spectra as lines. The Aladin preview contains a DSS image together with NVSS contours (blue) and the points and associated beams of the radio spectrum (red); points and beams of the sources from the waste basket are hidden but can be made visible by clicking on the corresponding plane (yellow).
VIII/85A/waste
Post annotation
SPECFIND V2.0 Catalog of radio continuum spectra (Vollmer+ 2009) [ReadMe+ftp]
Source parameters based on positional cross-id[spectrum] (1497216 rows)
img(gal)
start AladinLite

nu Name S(nu) e beam Seq RAJ2000 DEJ2000 MHz mJy mJy arcsec deg deg
74 VLSS J1449.2+3748 2.19e+03 4.4e+02 79.98 65273 222.3221 +37.8144 151 7C 144718.19+380105.00 1.27e+03 2.5e+02 70.20 65273 222.3212 +37.8114 232 MY 144718.1+374847.7 5.10e+02 1.0e+02 150.00 65273 222.3208 +37.8133 325 WN B1447.2+3801A 5.10e+01 1.0e+01 12.00 -65273 222.2923 +37.8505 325 WN B1447.2+3801B 6.07e+02 1.2e+02 12.00 65273 222.3211 +37.8122 365 TXS 1447+380 6.57e+02 1.3e+02 6.00 65273 222.3209 +37.8123 408 B2.3 1447+38 3.85e+02 7.7e+01 0.00 65273 222.3158 +37.8133 1400 FIRST J144909.3+375045 7.40e+00 1.5e+00 5.00 -65273 222.2891 +37.8459 1400 FIRST J144909.8+375102 1.71e+01 3.4e+00 5.00 -65273 222.2910 +37.8508 1400 FIRST J144916.8+374844 7.46e+01 1.5e+01 5.00 -65273 222.3202 +37.8124 1400 FIRST J144917.4+374841 4.08e+01 8.2e+00 5.00 -65273 222.3228 +37.8114 1400 NVSS J144909+375059 2.80e+01 5.6e+00 45.00 -65273 222.2909 +37.8499 4730 B3a 1447+380 2.80e+01 5.6e+00 168.00 65273 222.3212 +37.8151 4850 GB6 B1447+3801 3.78e+01 7.6e+00 108.00 65273 222.3117 +37.8222 10600 B3VLA 948 1.00e+01 2.0e+00 69.00 65273 222.3208 +37.8117

Note: For the spectrum finding algorithm, the errors have been increased by 50%